北京、郑州和深圳三城市空气中气溶胶单颗粒特征的扫描电镜分析   总被引：1，自引：0，他引：1  

赵承美  邵龙义  侯聪  幸娇萍  胡颖  王文华 《岩石矿物学杂志》2015,34(6):925-931

分别采集北京、深圳和郑州3个城市气溶胶样品,使用场发射扫锚电镜-能谱仪观察气溶胶单颗粒的显微形貌和元素组成,并利用图像分析系统对PM2.5的粒径进行了分析。结果表明,城市气溶胶单颗粒类型以矿物颗粒、烟尘和球形颗粒(飞灰和二次粒子)为主。对比3个城市气溶胶中不同颗粒类型数量百分比发现,矿物颗粒数量最多的城市是北京,飞灰和烟尘数量最多的城市是郑州,而规则矿物颗粒数量最多的城市是深圳。3个城市气溶胶单颗粒的数量-粒径分布均呈单峰分布。深圳气溶胶中颗粒物的粒径相对较小,其次为郑州、北京。3个城市气溶胶中颗粒物来源不同程度上都受到交通污染源影响,而燃煤源对北京和郑州气溶胶中颗粒物来源影响仍然不容忽视。  相似文献   

卵石地层的特殊性及其对基坑支护的影响分析     

刘伍  李海明 《城市地质》2015,(Z2)

主要从卵石地层的特征分类、特殊结构及场内施工条件3个方面,对基坑支护结构选型及施工工艺选择进行深入、系统的分析论证,力求使在卵石地层中的基坑支护设计方案更科学、经济,使施工方法、工艺更具可操作性。  相似文献   

Clinoform geometry,geomorphology, facies character and stratigraphic architecture of a sand‐rich subaqueous delta: Jurassic Sognefjord Formation,offshore Norway          下载免费PDF全文

Stefano Patruno  Gary J. Hampson  Christopher A.‐L. Jackson  Tom Dreyer 《Sedimentology》2015,62(1):350-388

The integration of core sedimentology, seismic stratigraphy and seismic geomorphology has enabled interpretation of delta‐scale (i.e. tens of metres high) subaqueous clinoforms in the upper Jurassic Sognefjord Formation of the Troll Field. Mud‐prone subaqueous deltas characterized by a compound clinoform morphology and sandy delta‐scale subaqueous clinoforms are common in recent tide‐influenced, wave‐influenced and current‐influenced settings, but ancient examples are virtually unknown. The data presented help to fully comprehend the criteria for the recognition of other ancient delta‐scale subaqueous clinoforms, as well as refining the depositional model of the reservoir in the super‐giant Troll hydrocarbon field. Two 10 to 60 m thick, overall coarsening‐upward packages are distinguished in the lower Sognefjord Formation. Progressively higher energy, wave‐dominated or current‐dominated facies occur from the base to the top of each package. Each package corresponds to a set of seismically resolved, westerly dipping clinoforms, the bounding surfaces of which form the seismic ‘envelope’ of a clinoform set and the major marine flooding surfaces recognized in cores. The packages thicken westwards, until they reach a maximum where the clinoform ‘envelope’ rolls over to define a topset–foreset–toeset geometry. All clinoforms are consistently oriented sub‐parallel to the edge of the Horda Platform (N005–N030). In the eastern half of the field, individual foresets are relatively gently dipping (1° to 6°) and bound thin (10 to 30 m) clinothems. Core data indicate that these proximal clinothems are dominated by fine‐grained, hummocky cross‐stratified sandstones. Towards the west, clinoforms gradually become steeper (5° to 14°) and bound thicker (15 to 60 m) clinothems that comprise medium‐grained, cross‐bedded sandstones. Topsets are consistently well‐developed, except in the westernmost area. No seismic or sedimentological evidence of subaerial exposure is observed. Deposition created fully subaqueous, near‐linear clinoforms that prograded westwards across the Horda Platform. Subaqueous clinoforms were probably fed by a river outlet in the north‐east and sculpted by the action of currents sub‐parallel to the clinoform strike.  相似文献   

新疆克拉玛依油田一中区克拉玛依组辫状河储层砂体类型及分布特征          下载免费PDF全文

杨婷  金振奎  张雷  赵坤  刘安 《沉积与特提斯地质》2015,(2):8-15

通过露头实测、岩心观察及测录井资料分析等结果表明,克拉玛依油田一中区克拉玛依组S7、S5和S4砂层组沉积时期以发育辫状河为特征,可进一步划分为近源砾质辫状河、远源砾质辫状河和砂质辫状河沉积3种类型。上述3种类型的辫状河沉积在沉积特征、河道空间叠置样式及组合关系等方面存在明显的差异。近源砾质辫状河河道岩性以砾岩为主,为中孔低渗储层。单河道沉积厚度2~4.5m,宽度500~800m,表现为河道-河道直接接触的连片组合方式;远源砾质辫状河河道岩性仍以砾岩为主,含少量砂岩,物性较近源砾质辫状河略好,为中孔低渗储层。单河道沉积厚度为1.5~4m,河道砂体宽度400~750m,表现为河道-溢岸-河道的连片组合方式;砂质辫状河河道岩性以砂岩为主,为中孔低渗储层,物性优于砾质辫状河。单层厚度为0.5~2.5m,宽度为300~700m,但河道沉积分布范围有限,河道之间多为带状或交织带状组合方式。根据上述对比分析认为砾质辫状河河道砂体虽然物性相对较差、非均质性较强,但砂体厚度大、分布广泛、连通性好,目前为全区主要油气开发的目的层;砂质辫状河河道砂体尽管物性较好,但由于厚度较薄,分布局限,仅在东部地区其累计厚度较大,当与其它成藏条件匹配时,可形成具有开发潜力的目的层。  相似文献   

深部细粒碎屑岩储层成岩作用研究——以苏北盆地张家垛油田阜三段为例          下载免费PDF全文

韩玫梅  丁晓琪  张哨楠  陈倩倩 《沉积与特提斯地质》2015,35(4):60-67

毗邻烃源岩的细粒储层,由于其岩石结构、组分及沉积环境的特殊性,成岩作用表现出一定差异。本文以张家垛油田阜三段细粒碎屑岩储层为例,通过铸体薄片、X射线衍射、扫描电镜等相关分析,研究其成岩作用的特殊性。研究结果表明:(1)细粒储层的成分成熟度和结构成熟度较高,常被泥岩包裹,在压实作用中若存在欠压实,粒间孔可以被很好地保留下来;(2)细粒储层形成时水动力较弱,杂基含量高导致微孔较多;(3)大量的粘土矿物使孔隙比表面增加,抑制了后期硅质和碳酸盐胶结物的析出;(4)比表面的增加减缓了孔隙流体的对流速率和扩散速率,不利于次生孔隙的形成,粒度越细,次生孔隙越不发育。细粒碎屑岩储层有别于常规储层,对其特殊的成岩作用进行研究具有重要的理论价值和实际意义。  相似文献   

A Method for Determining Sedimentary Micro-Facies Belts Automatically     

Linfu Xue  Qitai Mei  Quan Sun 《世界地质(英文版)》2003,6(1)

It is important to understand the distribution of sedimentary facies, especially the distribution of sand body that is the key for oil production and exploration. The secondary oil recovery requires analyzing a great deal of data accumulated within decades of oil field development. At many cases sedimentary micro-facies maps need to be reconstructed and redrawn frequently, which is time-consuming and heavy. This paper presents an integrated approach for determining the distribution of sedimentary micro-facies, tracing the micro-facies boundary, and drawing the map of sedimentary micro-facies belts automatically by computer technique. The approach is based on the division and correlation of strata of multiple wells as well as analysis of sedimentary facies. The approach includes transform, gridding, interpolation, superposing, searching boundary and drawing the map of sedimentary facies belts, and employs the spatial interpolation method and "worm" interpolation method to determine the distribution of sedimentary micro-facies including sand ribbon and/or sand blanket. The computer software developed on the basis of the above principle provides a tool for quick visualization and understanding the distribution of sedimentary micro-facies and reservoir. Satisfied results have been achieveed by applying the technique to the Putaohua Oil Field in Songliao Basin, China.  相似文献   

Models of the formation of the solar nebula     

Patrick Cassen  Audrey Summers 《Icarus》1983,53(1):26-40

Models of the collapse of a protostellar cloud and the formation of the solar nebula reveal that the size of the nebula produced will be the larger of $\text{R}{}_{\mathrm{<mtext>CF</mtext>}}\text{≡ J}{}^2\text{/k}{}^2\text{GM}{}^3\text{and}\text{R}{}_{\mathrm{<mtext>V</mtext>}}\text{≡ (GMv/2c}{}_{\mathrm{<mtext>c</mtext>}}{}^3\text{)}\text{1}\text{2}$ (where J, M, and c_s are the total angular momentum, total mass, and sound speed of the protosetellar material; G is the gravitational constant; k is a number of order unity; and v is the effective viscosity in the nebula). From this result it can be deduced that low-mass nebulas are produced if P ≡ (R_V/R_CF)² ? 1; “massive” nebulas result if P ? 1. Gravitational instabilities are expected to be important for the evolution of P ? 1 nebulas. The value of J distinguishes most current models of the solar nebula, since P ∝ J^?4. Analytic expressions for the surface density, nebular mass flux, and photospheric temperature distributions during the formation stage are presented for some simple models that illustrate the general properties of growing protostellar disks. It does not yet seem possible to rule out either P ? 1 or P < 1 for the solar nebula, but observed or possible heterogeneities in composition and angular-momentum orientation favor P < 1 models.  相似文献   

Analysis on the interplanetary causes of the great magnetic storms in solar maximum (2000-2001)     

X.H. Xue  Yuming Wang  P.Z. Ye  S. Wang  M. Xiong 《Planetary and Space Science》2005,53(4):443-457

In this paper, we analyze the interplanetary causes of eight great geomagnetic storms during the solar maximum (2000-2001). The result shows that the interplanetary causes were the intense southward magnetic field and the notable characteristic among the causal mechanism is compression. Six of eight great geomagnetic storms were associated with the compression of southward magnetic field, which can be classified into (1) the compression between ICMEs (2) the compression between ICMEs and interplanetary medium. It suggests that the compressed magnetic field would be more geoeffective. At the same time, we also find that half of all great storms were related to successive halo CMEs, most of which originated from the same active region. The interactions between successive halo CMEs usually can lead to greater geoeffectiveness by enhancing their southward field B_s interval either in the sheath region of the ejecta or within magnetic clouds (MCs). The types of them included: the compression between the fast speed transient flow and the slow speed background flow, the multiple MCs, besides shock compression. Further, the linear fit of the D_st versus gives the weights of and Δt as α=2.51 and β=0.75, respectively. This may suggest that the compression mechanism, with associated intense B_s, rather than duration, is the main factor in causing a great geomagnetic storm.  相似文献   

A field evaluation of enhanced reductive dechlorination of chlorinated solvents in groundwater,New York Metropolitan Area     

Eric?Rodriguez  Kevin?A.?McGuinness  Duke?U.?OphoriEmail author 《Environmental Geology》2004,45(5):623-632

An initial assessment of an old manufacturing site with groundwater impacted by trichloroethene (TCE) contamination in the metropolitan New York area showed that the TCE was being removed naturally by reductive dechlorination. However, complete dechlorination was not expected at the site because the process was progressing too slowly under transitional to aerobic conditions at a degradation constant of –0.0013 and a TCE half life of 533 days. A pilot test was conducted at the site in which a carbohydrate substrate (molasses) was injected into the groundwater to create an In-Situ Reactive Zone (IRZ). Post-pilot test groundwater sampling and analysis indicated that an IRZ was created successfully as the total organic carbon (TOC) content and conductivity increased significantly while oxidation-reduction (REDOX) potential and dissolved oxygen (DO) decreased. The created IRZ caused enhanced reductive dechlorination of TCE at the site, found to proceed with a degradation constant of –0.0158 and a TCE half life of 44 days.  相似文献   

玉林市“6·21”大暴雨成因分析     

陈明璐  张洁婷 《广西气象》2010,(4):34-36,48

利用常规的天气图、物理量场及数值预报等资料,对2010年6月21日玉林市出现的大暴雨天气进行分析,结果表明：（1）高空波动、中低层切变线、西南暖湿气流和地面弱冷空气是影响此次强降水过程的主要天气系统;（2）对于单站预报,在掌握大气环流形势背景的同时,综合分析各物理量场尤其是本站的重要物理量各层垂直分布,对预报有很好的指示意义。  相似文献